Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minute to calcaulte
Image
Pre-slew 15.0-350.0 keV image (Event data)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
50.4282 10.0076 0.0288 36.0172 -44.8161 0.3083608 6.678 TRIG_01101133
Foreground time interval of the image:
0.160 5.984 (delta_t = 5.824 [sec])
Background time interval of the image:
-79.027 0.160 (delta_t = 79.187 [sec])
Lightcurves
Notes:
- 1) The mask-weighted light curves are using the flight position.
- 2) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 3) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
- 4) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
- 5) Time of each bin is in the middle of the bin.
1 s binning
From T0-310 s to T0+310 s
From T100_start - 20 s to T100_end + 30 s
Full time interval
64 ms binning
Full time interval
From T100_start to T100_end
From T0-5 sec to T0+5 sec
16 ms binning
From T100_start-5 s to T100_start+5 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
8 ms binning
From T100_start-3 s to T100_start+3 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
2 ms binning
From T100_start-1 s to T100_start+1 s
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Quad-rate summed light curves (from T0-300s to T0+1000s)
Spectral Evolution
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) When the burst includes telescope slew time periods, the fitting uses an average response file made from multiple 5-s response files through out the slew time plus single time preiod for the non-slew times, and weighted by the total counts in the corresponding time period using addrmf. An average response file is needed becuase a spectral fit using the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
- 3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.
Time averaged spectrum fit using the average DRM
Power-law model
Time interval is from 0.160 sec. to 5.984 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.71215 ( -0.316365 0.333339 )
Norm@50keV : 4.02356E-03 ( -0.000861351 0.000840867 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.03 using 59 bins.
Reduced chi-squared = 0.807544
# Null hypothesis probability of 8.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 5.824 sec: 0.536685 ( -0.102165 0.10224 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.16796e-07 ( -4.74514e-08 4.87509e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.160 sec. to 5.984 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.133208 ( -2.64544 1.65337 )
Epeak [keV] : 51.6355 ( -12.5116 -51.4948 )
Norm@50keV : 3.02942E-02 ( -0.0314152 0.840997 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.40 using 59 bins.
Reduced chi-squared = 0.775
# Null hypothesis probability of 8.90e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 5.824 sec: 0.507251 ( -0.107432 0.107293 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.8893e-07 ( -4.69617e-08 5.56447e-08 ) ergs/cm2
Band function
Time interval is from 0.160 sec. to 5.984 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 12.0715 (-2.08662 2.61359)
R^2/D10^2 : 0.134519 (-0.0699992 0.136083)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.59 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.84e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 2.416e-08 8.541e-09
25- 50 7.656e-08 2.154e-08
50-150 6.734e-08 2.623e-08
15-150 1.681e-07 4.650e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 112.064 (-53.3801 -111.049)
Norm : 2.33730 (-0.499195 0.712451)
------------------------------------------------------------
#Fit statistic : Chi-Squared 44.61 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.84e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.553e-08 1.057e-08
25- 50 6.280e-08 3.337e-08
50-150 1.083e-07 7.616e-08
15-150 2.066e-07 1.288e-07
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 3.40605 (-3.41644 -3.41644)
R1^2/D10^2 : 5.22265 (-5.18131 -5.18131)
kT2 [keV] : 13.3385 (-2.72284 -13.3415)
R2^2/D10^2 : 8.67189E-02 (-0.0866331 0.130226)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.15 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.77e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.104e-08 1.504e-08
25- 50 7.008e-08 4.024e-08
50-150 7.696e-08 4.776e-08
15-150 1.781e-07 9.977e-08
Peak spectrum fit
Power-law model
Time interval is from 1.156 sec. to 2.156 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.73461 ( -0.400682 0.424281 )
Norm@50keV : 7.95755E-03 ( -0.0021662 0.00209577 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.73 using 59 bins.
Reduced chi-squared = 0.802281
# Null hypothesis probability of 8.58e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.07000 ( -0.253469 0.25361 ) ph/cm2/s
Energy fluence (15-150 keV) : 7.35072e-08 ( -2.0127e-08 2.08772e-08 ) ergs/cm2
Cutoff power-law model
Time interval is from 1.156 sec. to 2.156 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.17783 ( -2.36601 1.04014 )
Epeak [keV] : 62.4434 ( -51.7153 -62.4475 )
Norm@50keV : 1.67324E-02 ( -0.0167291 0.510946 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.31 using 59 bins.
Reduced chi-squared = 0.809107
# Null hypothesis probability of 8.46e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 1 sec: 1.05304 ( -0.256637 0.25722 ) ph/cm2/s
Energy fluence (15-150 keV) : 6.90987e-08 ( -2.2867e-08 2.34009e-08 ) ergs/cm2
Band function
Time interval is from 1.156 sec. to 2.156 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 9.92214 (-2.50408 4.00348)
R^2/D10^2 : 0.529565 (-0.380684 1.06134)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared 48.72 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 7.74e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.059e-08 4.938e-09
25- 50 2.604e-08 1.058e-08
50-150 1.328e-08 8.586e-09
15-150 4.991e-08 2.248e-08
Thermal bremsstrahlung (OTTB)
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 112.099 (-63.2308 -109.887)
Norm : 4.62317 (-1.25064 1.98004)
------------------------------------------------------------
#Fit statistic : Chi-Squared 45.31 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.68e-01 with 57 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.207e-08 7.030e-09
25- 50 2.133e-08 1.225e-08
50-150 3.678e-08 2.636e-08
15-150 7.018e-08 4.532e-08
Double BB
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 7.07945 (-2.32877 3.00761)
R1^2/D10^2 : 1.48832 (-1.06948 4.45041)
kT2 [keV] : 30.4273 (-25.8189 -30.5879)
R2^2/D10^2 : 6.17246E-03 (-0.00606557 0.0846633)
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.09 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.78e-01 with 55 degrees of freedom
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 1.301e-08 7.470e-09
25- 50 2.247e-08 1.281e-08
50-150 3.868e-08 2.224e-08
15-150 7.416e-08 3.790e-08
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 1.71215 ( -0.316365 0.333339 )
Norm@50keV : 4.02356E-03 ( -0.000861351 0.000840867 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 46.03 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.50e-01 with 57 degrees of freedom
Photon flux (15-150 keV) in 5.824 sec: 0.536661 ( -0.102159 0.102234 ) ph/cm2/s
Energy fluence (15-150 keV) : 2.16765e-07 ( -4.74109e-08 4.88089e-08 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 0.104822 ( -2.63438 1.66334 )
Epeak [keV] : 51.4733 ( -12.4871 -51.4721 )
Norm@50keV : 3.14641E-02 ( -0.0314729 0.840412 )
------------------------------------------------------------
#Fit statistic : Chi-Squared 43.40 using 59 bins.
Reduced chi-squared =
# Null hypothesis probability of 8.91e-01 with 56 degrees of freedom
Photon flux (15-150 keV) in 5.824 sec: 0.507205 ( -0.107416 0.107251 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.88986e-07 ( -4.69793e-08 5.57799e-08 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : ( )
beta : ( )
Epeak [keV] : ( )
Norm@50keV : ( )
------------------------------------------------------------
Photon flux (15-150 keV) in sec: ( ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 5.88e-08
S(50-100 keV) = 7.22e-08
T90 vs. Hardness ratio plot
T90 = 5.28000009059906 sec.
Hardness ratio (energy fluence ratio) = 1.22789
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 1.49136
Count Ratio (50-100 keV) / (15-25 keV) = 0.934638
Mask shadow pattern
IMX = 5.157150162567080E-01, IMY = 5.124147426178338E-01
TIME vs. PHA plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
TIME vs. DetID plot around the trigger time
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
100 us light curve (15-350 keV)
Blue+Cyan dotted lines: Time interval of the scaled map
From 0.000000 to 4.096000
Spacecraft aspect plot
Bright source in the pre-burst/pre-slew/post-slew images
Pre-burst image of 15-350 keV band
Time interval of the image:
-79.027410 0.160000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6393 22.0199 0.9 44.8 7.2 3.2857 12.9 0.5 Crab
96.7568 -18.2928 1.8 25.6 78.2 1.2565 6.5 ------ UNKNOWN
87.7215 -55.8113 2.0 37.7 152.2 1.5252 5.7 ------ UNKNOWN
65.2019 20.0533 2.7 40.9 -17.7 0.8975 4.3 ------ UNKNOWN
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.160000 5.984000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.7633 22.0954 7.9 44.9 7.3 -0.0827 -1.4 8.7 Crab
84.3811 -67.5624 2.1 47.8 161.2 0.4228 5.5 ------ UNKNOWN
83.9876 -34.6690 2.3 18.9 129.8 0.1593 5.1 ------ UNKNOWN
70.6306 5.7615 2.6 26.4 -9.2 0.1378 4.5 ------ UNKNOWN
66.5511 2.3224 2.3 23.2 -19.3 0.1441 5.0 ------ UNKNOWN
50.4282 10.0076 1.7 36.0 -44.8 0.3082 6.7 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
817.972600 962.737200
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
83.6231 22.0110 1.2 51.7 -159.1 5.4430 9.6 0.6 Crab
Plot creation:
Mon Oct 24 05:03:36 EDT 2022